Satoshi Honda
Astronomy and Astrophysics · 2002–2019
A researcher in the Science corpus: 13 papers; trusts 19 researchers and is trusted by 11 researchers here, as inferred from the citation graph.
Subfields
- Astronomy and Astrophysics — 206 citations into it; #4,695 of 10,964 by trust here, #3,026 by citations
- Instrumentation — 71 citations into it; #3,000 of 3,502 by trust here, #1,861 by citations
- Nuclear and High Energy Physics — 30 citations into it
- Mechanics of Materials — 8 citations into it
- Aerospace Engineering — 6 citations into it
Whom Satoshi Honda trusts overall
Their strongest outbound trust, strongest first, inferred from their citations.
- J. E. Lawler
- C. Sneden
- J. Cowan
- Wak Aoki
- E. A. Den Hartog
- Timothy C. Beers
- V. Hill
- Jennifer A. Johnson
- C. Pilachowski
- R. Cayrel
Who trusts Satoshi Honda overall
- Wak Aoki
- C. Sneden
- N. Nishimura
- Y. Qian
- J. Cowan
- Timothy C. Beers
- S. Wanajo
- Friedrich-Karl Thielemann
- Roberto Gallino
- A. Frebel
Papers from Satoshi Honda's perspective
Ordered by how strongly the researchers Satoshi Honda trusts endorse each paper. Same corpus, a different order for every researcher.
- Experimental Radiative Lifetimes, Branching Fractions, and Oscillator Strengths for La II and a New Determination of the Solar Lanthanum Abundance
- Improved Laboratory Transition Parameters forEu II and Application to the Solar Europium Elemental and Isotopic Composition
- Abundances of 30 Elements in 23 Metal-Poor Stars
- First stars. I. The extreme r-element rich, iron-poor halo giant CS 31082-001 - Implications for the r-process site(s) and radioactive cosmochronology
- First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- The Two Micron All Sky Survey (2MASS)
- The Rise of the s-Process in the Galaxy
- First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
- The Extremely Metal-poor, Neutron Capture-rich Star CS 22892-052: A Comprehensive Abundance Analysis
- The Chemical Composition and Age of the Metal-poor Halo Star BD +17°3248
Their papers
- Multi-messenger Observations of a Binary Neutron Star Merger (2019) — 3,158 citations
- Do Kepler Superflare Stars Really Include Slowly Rotating Sun-like Stars?—Results Using APO 3.5 m Telescope Spectroscopic Observations and Gaia-DR2 Data (2019) — 146 citations
- Kilonova from post-merger ejecta as an optical and near-infrared counterpart of GW170817 (2017) — 233 citations
- J-GEM observations of an electromagnetic counterpart to the neutron star merger GW170817 (2017) — 179 citations
- Statistical properties of superflares on solar-type stars based on 1-min cadence data (2015) — 189 citations
- SUPERFLARES ON SOLAR-TYPE STARS OBSERVED WITH KEPLER. I. STATISTICAL PROPERTIES OF SUPERFLARES (2013) — 382 citations
- HIGH-RESOLUTION SPECTROSCOPY OF EXTREMELY METAL-POOR STARS FROM SDSS/SEGUE. I. ATMOSPHERIC PARAMETERS AND CHEMICAL COMPOSITIONS (2012) — 144 citations
- Can Superflares Occur on Our Sun (2012) — 205 citations
- Neutron-Capture Elements in the Very Metal Poor Star HD 122563 (2006) — 179 citations
- Spectroscopic Studies of Very Metal-poor Stars with the Subaru High Dispersion Spectrograph. III. Light Neutron-Capture Elements (2005) — 158 citations
- HE 1327–2326, an Unevolved Star with [Fe/H] < –5.0. I. A Comprehensive Abundance Analysis (2005) — 165 citations
- Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. II. The r-Process Elements, Including Thorium (2004) — 286 citations
- High Dispersion Spectrograph (HDS) for the Subaru Telescope (2002) — 298 citations